{"id":519875,"date":"2026-08-26T02:13:49","date_gmt":"2026-08-25T16:13:49","guid":{"rendered":"https:\/\/science.nasa.gov\/missions\/chandra\/galactic-gems-glisten-in-new-gallery-from-nasas-chandra\/"},"modified":"2026-08-26T02:13:49","modified_gmt":"2026-08-25T16:13:49","slug":"galactic-gems-glisten-in-new-gallery-from-nasas-chandra","status":"publish","type":"post","link":"https:\/\/www.vibewire.com.au\/?p=519875","title":{"rendered":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra"},"content":{"rendered":"<div id=\"\" class=\"hds-article-hero-header nasa-gb-align-full bg-carbon-90 width-full maxw-full color-mode-dark hds-module hds-module-full alignfull wp-block-nasa-blocks-article-hero-header\">\n<div class=\"hds-cover-wrapper width-full maxw-full minh-tablet grid-container minh-tablet flex-column padding-0\">\n<div class=\"hds-foreground-wrapper display-flex flex-direction-column\">\n<div class=\"grid-container grid-container-block margin-top-auto width-full maxw-desktop-lg padding-y-9 padding-x-3 desktop:padding-x-3 z-400\">\n<div class=\"z-400 grid-col-12 tablet:grid-col-12 desktop:grid-col-7 z-400\">\n<div class=\"margin-0\">\n<div class=\"label color-spacesuit-white margin-bottom-2\">4 Min Read<\/div>\n<h1 class=\"heading-41 line-height-md color-spacesuit-white-important\">\n\t\t\t\t\t\t\t\tGalactic Gems Glisten in New Gallery From NASA\u2019s Chandra\t\t\t\t\t\t\t<\/h1>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 tablet:grid-col-12 desktop:grid-col-5\"><\/div>\n<div class=\"skrim-overlay skrim-left mobile-skrim-top z-200\"><\/div>\n<figure class=\"hds-media-background  \"><img fetchpriority=\"high\" decoding=\"async\" width=\"4336\" height=\"2794\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"A spiral galaxy viewed from its side, featuring a giant halo of hot gas blowing out of its stellar disk. X-rays from Chandra and ESA\u2019s XMM-Newton (purple and royal blue) trace hot gas driven out by supernovas and black holes and neutron stars pulling gas from their companions, while optical light (light blue, gold and white) from ground-based observer R. Jay GaBany showcases dense dust lanes. Edge-on views of galaxies allow astronomers to study how flat their stellar disks are and provide the clearest views of material located above or below the disk.\" style=\"transform: scale(1); transform-origin: 0% 42%; object-position: 0% 42%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"eager\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&#038;fit=crop&#038;crop=faces%2Cfocalpoint 4336w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=300&#038;h=193&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=768&#038;h=495&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1024&#038;h=660&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1536&#038;h=990&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=2048&#038;h=1320&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=400&#038;h=258&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=600&#038;h=387&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=900&#038;h=580&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1200&#038;h=773&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=2000&#038;h=1289&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 4336px) 100vw, 4336px\" \/><\/figure>\n<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\">Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety.<\/p>\n<p class=\"wp-block-paragraph\">Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating from their cores, ellipticals that are older and likely the results of mergers, and irregulars that can encompass a wide range of galactic phenomena.<\/p>\n<div id=\"\" class=\"hds-media hds-module wp-block-image\">\n<div class=\"margin-left-auto margin-right-auto nasa-block-align-inline\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-fit \" style=\"--hds-image-contain-bg:#ffffff;\"><a href=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=6000&#038;h=4364&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" rel=\"noopener\"><img decoding=\"async\" width=\"6000\" height=\"4364\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=6000&#038;h=4364&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-2048x2048 size-2048x2048\" alt=\"This gallery displays a collection of 16 galactic images from Chandra and other telescopes. Astronomers put galaxies into three main categories: spirals like our own Milky Way, ellipticals that are older and likely the results of mergers, and irregulars that can encompass a wide range of galactic phenomena. All types are represented in this collection. Each galactic image contains X-ray data from Chandra combined with data from telescopes such as NASA\u2019s Webb, Hubble, IXPE, Swift, and NuSTAR, and others both in space and on the ground.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=6000&#038;h=4364&#038;fit=crop&#038;crop=faces%2Cfocalpoint 6000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=300&#038;h=218&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=768&#038;h=559&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=1024&#038;h=745&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=1536&#038;h=1117&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=2048&#038;h=1490&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=400&#038;h=291&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=600&#038;h=436&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=900&#038;h=655&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=1200&#038;h=873&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_labeled.jpg?w=2000&#038;h=1455&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 6000px) 100vw, 6000px\" \/><\/a><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-caption-text p-sm margin-0\">This gallery displays a collection of 16 galactic images from Chandra and other telescopes. Astronomers put galaxies into three main categories: spirals like our own Milky Way, ellipticals that are older and likely the results of mergers, and irregulars that can encompass a wide range of galactic phenomena. All types are represented in this collection. Each galactic image contains X-ray data from Chandra combined with data from telescopes such as NASA\u2019s Webb, Hubble, IXPE, Swift, and NuSTAR, and others both in space and on the ground.<\/div>\n<div class=\"hds-credits\">Credit: NASA\/CXC\/SAO<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n<p class=\"has-text-align-left wp-block-paragraph\"><a href=\"https:\/\/science.nasa.gov\/gallery\/galaxy-gallery-galactic-gems-glisten-in-new-gallery-from-nasas-chandra\/\" rel=\"noopener\"><strong>See full gallery<\/strong><\/a><\/p>\n<p class=\"wp-block-paragraph\">Just as gems reveal the history of Earth through how they were forged over billions of years, these galactic gems are a way to study Earth\u2019s place in our home galaxy of the Milky Way. By looking outward to other galaxies, we learn more about our own \u2013 including clues to its past and future.<\/p>\n<p class=\"wp-block-paragraph\">There are 16 new images in this galactic gallery. Each one contains X-ray data from Chandra that has been collected across Chandra\u2019s decades in space. This high-energy data has been combined with data from telescopes such as NASA\u2019s James Webb and Hubble Space Telescopes, IXPE (Imaging X-ray Polarimetry Explorer), Neil Gehrels Swift Observatory, NuSTAR (Nuclear Spectroscopic Telescope Array), and others both on the ground and in space.<\/p>\n<div id=\"\" class=\"hds-image-carousel grid-container grid-container-block padding-top-4 padding-bottom-4 hds-module hds-module-full alignfull wp-block-nasa-blocks-image-carousel\">\n<div id=\"carousel-wrapper-carousel-6a8dc55763854\" class=\"hds-carousel-wrapper\">\n<div class=\"image-carousel-slider margin-0\" id=\"image-carousel-slider-carousel-6a8dc55763854\"\n\t\t\t\tdata-client-id=\"carousel-6a8dc55763854\"\n\t\t\t\tdata-variation=\"carousel\"\n\t\t\t\tdata-autoplay=\"\" \n\t\t\t\tdata-autoplay-speed=\"2000\" \n\t\t\t\tdata-play-pause=\"\" \n\t\t\t\tdata-transition-type=\"slide\"\n\t\t\t\tdata-progress=\"\"\n\t\t\t\tdata-progress-labels=\"\"\n\t\t\t\tdata-start-label=\"Start\"\n\t\t\t\tdata-end-label=\"End\"\n\t\t\t\tdata-labels-initialized=\"true\"><\/p>\n<div class=\"display-block width-full\" data-label=\"NGC 1672\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3000\" height=\"2133\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=3000&#038;h=2133&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A barred spiral galaxy featuring a prominent central bar or bridge of stars that channels gas toward its core. Chandra X-rays (purple) highlight growing black holes along the bar and core, merged with Hubble optical light (white, yellow and soft blue) and JWST infrared dust filaments (red). Studying barred spirals in action can help reveal how gas in our own Milky Way, which is also a barred spiral, feeds its central black hole and forms new stars.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=3000&#038;h=2133&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=300&#038;h=213&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=768&#038;h=546&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=1024&#038;h=728&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=1536&#038;h=1092&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=2048&#038;h=1456&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=400&#038;h=284&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=600&#038;h=427&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=900&#038;h=640&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=1200&#038;h=853&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1672.jpg?w=2000&#038;h=1422&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 1672<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A barred spiral galaxy featuring a prominent central bar or bridge of stars that channels gas toward its core. Chandra X-rays (purple) highlight growing black holes along the bar and core, merged with Hubble optical light (white, yellow and soft blue) and JWST infrared dust filaments (red). Studying barred spirals in action can help reveal how gas in our own Milky Way, which is also a barred spiral, feeds its central black hole and forms new stars.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI\/Hubble Heritage Team; Infrared: NASA\/ESA\/CSA\/STScI\/J. Lee and T. Williams; Image Processing: NASA\/CXC\/SAO\/L. Frattare, J. Major, K. Arcand<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"II Zw 096\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3600\" height=\"2644\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=3600&#038;h=2644&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A chaotic, dust-shrouded system of merging galaxies forming stars at a furious rate. Chandra X-ray data (magenta) pinpoint powerful black hole activity and hot gas, while Hubble optical (blue and white) and Webb infrared (red and grey) data illuminate vast stellar nurseries hidden behind interstellar dust. Systems like II Zw 096 show us how powerful galaxy collisions shaped the early universe.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=3600&#038;h=2644&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=300&#038;h=220&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=768&#038;h=564&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=1024&#038;h=752&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=1536&#038;h=1128&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=2048&#038;h=1504&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=400&#038;h=294&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=600&#038;h=441&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=900&#038;h=661&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=1200&#038;h=881&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_iizw096.jpg?w=2000&#038;h=1469&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3600px) 100vw, 3600px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">II Zw 096<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A chaotic, dust-shrouded system of merging galaxies forming stars at a furious rate. Chandra X-ray data (magenta) pinpoint powerful black hole activity and hot gas, while Hubble optical (blue and white) and Webb infrared (red and grey) data illuminate vast stellar nurseries hidden behind interstellar dust. Systems like II Zw 096 show us how powerful galaxy collisions shaped the early universe.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare and J. Major<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"M33\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"4050\" height=\"3397\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=4050&#038;h=3397&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A nearby, face-on spiral galaxy whose clear spiral arms offer an unhindered view of its stellar engine. X-ray data from Chandra (purple) highlights point sources like neutron stars and stellar-mass black holes pulling material off companion stars (systems called X-ray binaries), while optical data from the Very Large Telescope\u2019s MUSE instrument (pink and grey) maps glowing pockets of hydrogen gas. Ultraviolet data from NASA\u2019s Swift telescope (blue) reveals populations of young, massive stars sizzling across the spiral arms. M33\u2019s proximity to us allows astronomers to audit individual high-energy objects and map how stellar feedback affects a galaxy's ecosystem.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=4050&#038;h=3397&#038;fit=crop&#038;crop=faces%2Cfocalpoint 4050w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=300&#038;h=252&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=768&#038;h=644&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=1024&#038;h=859&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=1536&#038;h=1288&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=2048&#038;h=1718&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=400&#038;h=336&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=600&#038;h=503&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=900&#038;h=755&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=1200&#038;h=1007&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m33.jpg?w=2000&#038;h=1678&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 4050px) 100vw, 4050px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">M33<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A nearby, face-on spiral galaxy whose clear spiral arms offer an unhindered view of its stellar engine. X-ray data from Chandra (purple) highlights point sources like neutron stars and stellar-mass black holes pulling material off companion stars (systems called X-ray binaries), while optical data from the Very Large Telescope\u2019s MUSE instrument (pink and grey) maps glowing pockets of hydrogen gas. Ultraviolet data from NASA\u2019s Swift telescope (blue) reveals populations of young, massive stars sizzling across the spiral arms. M33\u2019s proximity to us allows astronomers to audit individual high-energy objects and map how stellar feedback affects a galaxy\u2019s ecosystem.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: ESO\/VLT; UV: NASA\/Swift; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 4258\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"4968\" height=\"3797\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=4968&#038;h=3797&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A spiral galaxy famous for having two extra, \"anomalous\" spiral arms composed of hot gas. Chandra's X-rays (royal blue) show superheated shockwaves created by central black hole jets, combined with optical light from Hubble (red, yellow and pale blue) and infrared dust filaments from Webb (bright orange). M106 helps show how supermassive black holes can create structural features that mimic star-bearing spiral arms, influencing a galaxy's evolution.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=4968&#038;h=3797&#038;fit=crop&#038;crop=faces%2Cfocalpoint 4968w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=300&#038;h=229&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=768&#038;h=587&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=1024&#038;h=783&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=1536&#038;h=1174&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=2048&#038;h=1565&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=400&#038;h=306&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=600&#038;h=459&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=900&#038;h=688&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=1200&#038;h=917&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4258.jpg?w=2000&#038;h=1529&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 4968px) 100vw, 4968px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 4258<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A spiral galaxy famous for having two extra, \u201canomalous\u201d spiral arms composed of hot gas. Chandra\u2019s X-rays (royal blue) show superheated shockwaves created by central black hole jets, combined with optical light from Hubble (red, yellow and pale blue) and infrared dust filaments from Webb (bright orange). M106 helps show how supermassive black holes can create structural features that mimic star-bearing spiral arms, influencing a galaxy\u2019s evolution.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 1569\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3000\" height=\"2013\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=3000&#038;h=2013&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A compact dwarf irregular galaxy undergoing a violent, compact burst of star formation. Chandra and XMM-Newton observations (blue and purple) reveal massive bubbles of million-degree gas inflated by stellar winds, set against a backdrop of optical light (magenta, orange and white) imaged by Adam Block. Dwarf starburst galaxies can serve as local laboratories for studying the conditions of the early universe, where small, primitive galaxies formed stars at frantic rates.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=3000&#038;h=2013&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=300&#038;h=201&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=768&#038;h=515&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=1024&#038;h=687&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=1536&#038;h=1031&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=2048&#038;h=1374&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=400&#038;h=268&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=600&#038;h=403&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=900&#038;h=604&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=1200&#038;h=805&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1569.jpg?w=2000&#038;h=1342&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 1569<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A compact dwarf irregular galaxy undergoing a violent, compact burst of star formation. Chandra and XMM-Newton observations (blue and purple) reveal massive bubbles of million-degree gas inflated by stellar winds, set against a backdrop of optical light (magenta, orange and white) imaged by Adam Block. Dwarf starburst galaxies can serve as local laboratories for studying the conditions of the early universe, where small, primitive galaxies formed stars at frantic rates.<\/div>\n<div class=\"hds-credits\">X-ray: (XMM):ESA\/XMM-Newton, (Chandra): NASA\/CXC\/SAO; Optical: Univ.of Arizona\/Mt Lemmon SkyCenter\/Adam Block\/Josep Drudis; Image Processing: NASA?CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"M90\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"4500\" height=\"4156\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=4500&#038;h=4156&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A large spiral galaxy that is being stripped of its gas as it plunges at high speed through hot gas in the Virgo Cluster of galaxies. Chandra\u2019s X-ray data (magenta) pinpoints high-energy point sources\u2014such as X-ray binaries and supernova remnants\u2014and diffuse hot gas nestled within the spiral disk imaged by Hubble (blue, brown and gold). A ground-based optical light image taken from New Mexico by Timothy Martin reveals red filaments of hydrogen gas streaming over 300,000 light-years behind the galaxy as it falls into the Virgo Cluster.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=4500&#038;h=4156&#038;fit=crop&#038;crop=faces%2Cfocalpoint 4500w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=300&#038;h=277&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=768&#038;h=709&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=1024&#038;h=946&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=1536&#038;h=1419&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=2048&#038;h=1891&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=400&#038;h=369&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=600&#038;h=554&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=900&#038;h=831&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=1200&#038;h=1108&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m90_fullfield.jpg?w=2000&#038;h=1847&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 4500px) 100vw, 4500px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">M90<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A large spiral galaxy that is being stripped of its gas as it plunges at high speed through hot gas in the Virgo Cluster of galaxies. Chandra\u2019s X-ray data (magenta) pinpoints high-energy point sources\u2014such as X-ray binaries and supernova remnants\u2014and diffuse hot gas nestled within the spiral disk imaged by Hubble (blue, brown and gold). A ground-based optical light image taken from New Mexico by Timothy Martin reveals red filaments of hydrogen gas streaming over 300,000 light-years behind the galaxy as it falls into the Virgo Cluster.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/D. Thilker\/J. Lee\/PHANGS-HST Team; Full-field: Tim Martin; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"Centaurus A\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3600\" height=\"3600\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=3600&#038;h=3600&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A giant elliptical galaxy undergoing a dusty merger, featuring a powerful jet of particles blasting tens of thousands of light-years into space. Chandra\u2019s X-rays (blue) showcase the high-energy jet, with additional X-rays from IXPE (orange), while Webb infrared (magenta) and optical light (amber and white) from the European Southern Observatory expose a dark, churning dust lane. As one of the closest active galaxies to Earth, Cen A allows astronomers to study the effects of supermassive black hole jets in extraordinary detail.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=3600&#038;h=3600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=150&#038;h=150&#038;fit=crop&#038;crop=faces%2Cfocalpoint 150w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=300&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=768&#038;h=768&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=1024&#038;h=1024&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=1536&#038;h=1536&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=2048&#038;h=2048&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=50&#038;h=50&#038;fit=crop&#038;crop=faces%2Cfocalpoint 50w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=100&#038;h=100&#038;fit=crop&#038;crop=faces%2Cfocalpoint 100w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=200&#038;h=200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=400&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=600&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=900&#038;h=900&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=1200&#038;h=1200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_cena.jpg?w=2000&#038;h=2000&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3600px) 100vw, 3600px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">Centaurus A<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A giant elliptical galaxy undergoing a dusty merger, featuring a powerful jet of particles blasting tens of thousands of light-years into space. Chandra\u2019s X-rays (blue) showcase the high-energy jet, with additional X-rays from IXPE (orange), while Webb infrared (magenta) and optical light (amber and white) from the European Southern Observatory expose a dark, churning dust lane. As one of the closest active galaxies to Earth, Cen A allows astronomers to study the effects of supermassive black hole jets in extraordinary detail.<\/div>\n<div class=\"hds-credits\">X-ray: (Chandra) NASA\/CXC\/SAO, X-ray (IXPE): NASA\/MSFC; Optical: ESO; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare, K. Arcand, and J. Major<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"M104\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"6000\" height=\"3737\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=6000&#038;h=3737&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"Famous for its broad central bulge and dark outer dust ring, this galaxy sits at a nearly edge-on tilt to Earth. Chandra X-rays (cyan and orange) isolate compact point sources and hot gas in the galaxy's sprawling halo, merged with Hubble optical light (warm white) and Webb infrared vision (purple-red dust lane). Studying M104 may help bridge the gap between spirals and ellipticals, helping astronomers better understand how a galaxy's giant outer cloud of stars grows and ages alongside its inner disk.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=6000&#038;h=3737&#038;fit=crop&#038;crop=faces%2Cfocalpoint 6000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=300&#038;h=187&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=768&#038;h=478&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=1024&#038;h=638&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=1536&#038;h=957&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=2048&#038;h=1276&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=400&#038;h=249&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=600&#038;h=374&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=900&#038;h=561&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=1200&#038;h=747&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m104.jpg?w=2000&#038;h=1246&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 6000px) 100vw, 6000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">M104<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">Famous for its broad central bulge and dark outer dust ring, this galaxy sits at a nearly edge-on tilt to Earth. Chandra X-rays (cyan and orange) isolate compact point sources and hot gas in the galaxy\u2019s sprawling halo, merged with Hubble optical light (warm white) and Webb infrared vision (purple-red dust lane). Studying M104 may help bridge the gap between spirals and ellipticals, helping astronomers better understand how a galaxy\u2019s giant outer cloud of stars grows and ages alongside its inner disk.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical:NASA\/Hubble Heritage Team\/AURA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"Arp 143\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3300\" height=\"2147\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=3300&#038;h=2147&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"This ring galaxy system formed when a smaller companion galaxy punched straight through its center like a bullseye, creating a powerful cosmic shockwave. Chandra X-rays (purple) uncover bright X-ray binary systems scattered along the collision shock wave, laid over Hubble\u2019s optical image (blue and white) of expanding stellar rings. Such head-on collisions can trigger vast ripple effects, sparking huge waves of star birth across entire galaxies.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=3300&#038;h=2147&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=300&#038;h=195&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=768&#038;h=500&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=1024&#038;h=666&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=1536&#038;h=999&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=2048&#038;h=1332&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=400&#038;h=260&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=600&#038;h=390&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=900&#038;h=586&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=1200&#038;h=781&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_arp143.jpg?w=2000&#038;h=1301&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3300px) 100vw, 3300px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">Arp 143<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">This ring galaxy system formed when a smaller companion galaxy punched straight through its center like a bullseye, creating a powerful cosmic shockwave. Chandra X-rays (purple) uncover bright X-ray binary systems scattered along the collision shock wave, laid over Hubble\u2019s optical image (blue and white) of expanding stellar rings. Such head-on collisions can trigger vast ripple effects, sparking huge waves of star birth across entire galaxies.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI\/J. Dalcanton; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 4725\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3000\" height=\"2279\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=3000&#038;h=2279&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A \"one-armed\" barred spiral galaxy surrounded by a prominent star-forming ring. Chandra's X-ray data (magenta) pinpoints several bright X-ray sources, likely caused by growing black holes, embedded within the sweeping optical disk (soft blue and white) captured with the Mt. Lemmon Observatory. Galaxies with unusual single arms can offer a window into how the gravity from a passing galaxy can trigger bursts of star formation.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=3000&#038;h=2279&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=300&#038;h=228&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=768&#038;h=583&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=1024&#038;h=778&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=1536&#038;h=1167&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=2048&#038;h=1556&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=400&#038;h=304&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=600&#038;h=456&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=900&#038;h=684&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=1200&#038;h=912&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4725.jpg?w=2000&#038;h=1519&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 4725<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A \u201cone-armed\u201d barred spiral galaxy surrounded by a prominent star-forming ring. Chandra\u2019s X-ray data (magenta) pinpoints several bright X-ray sources, likely caused by growing black holes, embedded within the sweeping optical disk (soft blue and white) captured with the Mt. Lemmon Observatory. Galaxies with unusual single arms can offer a window into how the gravity from a passing galaxy can trigger bursts of star formation.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI\/NAOJ\/R. Gendler; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 1385\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3600\" height=\"2702\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=3600&#038;h=2702&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A barred spiral galaxy packed with regions where stars are actively forming. Chandra X-ray data (magenta) highlights stellar nurseries and X-ray binaries scattered along dusty spiral structures brought to life by Hubble optical (white and grey) and Webb infrared (orange and red) observations. Comparing multiwavelength data of barred spirals containing active star formation helps scientists map how local starbursts build up galactic mass over time.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=3600&#038;h=2702&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=300&#038;h=225&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=768&#038;h=576&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=1024&#038;h=769&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=1536&#038;h=1153&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=2048&#038;h=1537&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=400&#038;h=300&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=600&#038;h=450&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=900&#038;h=676&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=1200&#038;h=901&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc1385.jpg?w=2000&#038;h=1501&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3600px) 100vw, 3600px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 1385<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A barred spiral galaxy packed with regions where stars are actively forming. Chandra X-ray data (magenta) highlights stellar nurseries and X-ray binaries scattered along dusty spiral structures brought to life by Hubble optical (white and grey) and Webb infrared (orange and red) observations. Comparing multiwavelength data of barred spirals containing active star formation helps scientists map how local starbursts build up galactic mass over time.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 660\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3000\" height=\"2343\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=3000&#038;h=2343&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A rare \"polar ring\" galaxy where a tilted outer ring of stars and dust rotates over the galaxy's poles, an unusual structure likely caused by a collision with another galaxy about a billion years ago. Chandra\u2019s X-rays (purple) reveal a possible growing supermassive black hole in the center of the galaxy, plus X-ray binaries nestled within the stars and dust captured by the Gemini Observatory in optical light (gold, blue and white). Studying polar rings teaches us about the diverse effects of stellar collisions on the shapes of galaxies.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=3000&#038;h=2343&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=300&#038;h=234&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=768&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=1024&#038;h=800&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=1536&#038;h=1200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=2048&#038;h=1599&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=400&#038;h=312&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=600&#038;h=469&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=900&#038;h=703&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=1200&#038;h=937&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc660.jpg?w=2000&#038;h=1562&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 660<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A rare \u201cpolar ring\u201d galaxy where a tilted outer ring of stars and dust rotates over the galaxy\u2019s poles, an unusual structure likely caused by a collision with another galaxy about a billion years ago. Chandra\u2019s X-rays (purple) reveal a possible growing supermassive black hole in the center of the galaxy, plus X-ray binaries nestled within the stars and dust captured by the Gemini Observatory in optical light (gold, blue and white). Studying polar rings teaches us about the diverse effects of stellar collisions on the shapes of galaxies.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical:NSF\/International Gemini Observatory\/AURA; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"M82\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"5688\" height=\"4551\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=5688&#038;h=4551&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"An irregular galaxy undergoing intense star formation because of a gravitational interaction with a neighboring galaxy hundreds of millions of years ago. Chandra X-rays (blue), supplemented by NuSTAR data, show towering superwinds of million-degree gas blowing thousands of light-years out of the galactic disk, with Hubble optical light (yellow, orange and white) showing the galaxy shape, and Webb and Spitzer detailing infrared dust emission (red). M82 was nicknamed the Cigar Galaxy mostly because of its edge-on angle to Earth, which makes its central disk look like an elongated, cigar-shaped oval with small optical telescopes. The galaxy illustrates how violent galactic \"exhaust systems\" can regulate a galaxy's growth by venting gas outwards.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=5688&#038;h=4551&#038;fit=crop&#038;crop=faces%2Cfocalpoint 5688w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=300&#038;h=240&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=768&#038;h=614&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=1024&#038;h=819&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=1536&#038;h=1229&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=2048&#038;h=1639&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=400&#038;h=320&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=600&#038;h=480&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=900&#038;h=720&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=1200&#038;h=960&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_m82.jpg?w=2000&#038;h=1600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 5688px) 100vw, 5688px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">M82<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">An irregular galaxy undergoing intense star formation because of a gravitational interaction with a neighboring galaxy hundreds of millions of years ago. Chandra X-rays (blue), supplemented by NuSTAR data, show towering superwinds of million-degree gas blowing thousands of light-years out of the galactic disk, with Hubble optical light (yellow, orange and white) showing the galaxy shape, and Webb and Spitzer detailing infrared dust emission (red). M82 was nicknamed the Cigar Galaxy mostly because of its edge-on angle to Earth, which makes its central disk look like an elongated, cigar-shaped oval with small optical telescopes. The galaxy illustrates how violent galactic \u201cexhaust systems\u201d can regulate a galaxy\u2019s growth by venting gas outwards.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare, J. Major, and K. Arcand<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 3256\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3813\" height=\"3447\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=3813&#038;h=3447&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A pair of colliding, gas-rich spiral galaxies merging into a single massive system. Chandra\u2019s X-ray data (pink) isolates point sources and shock-heated gas, Hubble\u2019s optical light (blue and white) captures tidal tails of stars, and Webb\u2019s infrared vision (red and orange) cuts through the dust to show hidden star formation. Galaxy collisions like this offer a preview of our far future, showing what might happen if our own Milky Way collides and merges with the nearby Andromeda Galaxy.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=3813&#038;h=3447&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3813w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=300&#038;h=271&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=768&#038;h=694&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=1024&#038;h=926&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=1536&#038;h=1389&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=2048&#038;h=1851&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=400&#038;h=362&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=600&#038;h=542&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=900&#038;h=814&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=1200&#038;h=1085&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3256.jpg?w=2000&#038;h=1808&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3813px) 100vw, 3813px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 3256<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A pair of colliding, gas-rich spiral galaxies merging into a single massive system. Chandra\u2019s X-ray data (pink) isolates point sources and shock-heated gas, Hubble\u2019s optical light (blue and white) captures tidal tails of stars, and Webb\u2019s infrared vision (red and orange) cuts through the dust to show hidden star formation. Galaxy collisions like this offer a preview of our far future, showing what might happen if our own Milky Way collides and merges with the nearby Andromeda Galaxy.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: NASA\/ESA\/STScI; Infrared: NASA\/ESA\/CSA\/STScI; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 3938\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"3000\" height=\"2819\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=3000&#038;h=2819&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A face-on spiral galaxy whose orientation gives us an unobstructed view of its disk. X-ray emissions from Chandra (magenta) detail energetic X-ray binaries and supernova remnants scattered across dust lanes in an optical image (white, blue and gold) from Adam Block with Mt. Lemmon Observatory. Face-on orientations are important for galactic studies because they provide the most unobstructed views of a galaxy\u2019s stars and gas.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=3000&#038;h=2819&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=300&#038;h=282&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=768&#038;h=722&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=1024&#038;h=962&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=1536&#038;h=1443&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=2048&#038;h=1924&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=400&#038;h=376&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=600&#038;h=564&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=900&#038;h=846&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=1200&#038;h=1128&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc3938.jpg?w=2000&#038;h=1879&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 3938<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A face-on spiral galaxy whose orientation gives us an unobstructed view of its disk. X-ray emissions from Chandra (magenta) detail energetic X-ray binaries and supernova remnants scattered across dust lanes in an optical image (white, blue and gold) from Adam Block with Mt. Lemmon Observatory. Face-on orientations are important for galactic studies because they provide the most unobstructed views of a galaxy\u2019s stars and gas.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: Adam Block\/Mount Lemmon SkyCenter\/University of Arizona; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<div class=\"display-block width-full\" data-label=\"NGC 4631\">\n<figure class=\"margin-0\">\n<div class=\"hds-cover-wrapper hds-image-carousel-slide margin-bottom-2 hds-object-fit-contain\">\n<div class=\"hds-media-wrapper margin-left-auto margin-right-auto\">\n<figure class=\"hds-media-inner hds-cover-wrapper hds-media-ratio-cover \"><img decoding=\"async\" width=\"4336\" height=\"2794\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-large size-large\" alt=\"A spiral galaxy viewed from its side, featuring a giant halo of hot gas blowing out of its stellar disk. X-rays from Chandra and ESA\u2019s XMM-Newton (purple and royal blue) trace hot gas driven out by supernovas and black holes and neutron stars pulling gas from their companions, while optical light (light blue, gold and white) from ground-based observer R. Jay GaBany showcases dense dust lanes. Edge-on views of galaxies allow astronomers to study how flat their stellar disks are and provide the clearest views of material located above or below the disk.\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&#038;fit=crop&#038;crop=faces%2Cfocalpoint 4336w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=300&#038;h=193&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=768&#038;h=495&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1024&#038;h=660&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1536&#038;h=990&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=2048&#038;h=1320&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=400&#038;h=258&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=600&#038;h=387&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=900&#038;h=580&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=1200&#038;h=773&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=2000&#038;h=1289&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 4336px) 100vw, 4336px\" \/><\/figure><figcaption class=\"hds-caption padding-y-2\">\n<div class=\"hds-date-text p-sm margin-0\">NGC 4631<\/div>\n<div class=\"hds-caption-text p-sm margin-0\">A spiral galaxy viewed from its side, featuring a giant halo of hot gas blowing out of its stellar disk. X-rays from Chandra and ESA\u2019s XMM-Newton (purple and royal blue) trace hot gas driven out by supernovas and black holes and neutron stars pulling gas from their companions, while optical light (light blue, gold and white) from ground-based observer R. Jay GaBany showcases dense dust lanes. Edge-on views of galaxies allow astronomers to study how flat their stellar disks are and provide the clearest views of material located above or below the disk.<\/div>\n<div class=\"hds-credits\">X-ray: NASA\/CXC\/SAO; Optical: \u00a92011-2015 by R Jay GaBany, Cosmotography.com; Image Processing: NASA\/CXC\/SAO\/L. Frattare<\/div>\n<\/figcaption><\/div>\n<\/p>\n<\/div>\n<\/figure>\n<\/div>\n<\/div>\n<div class=\"hds-carousel-nav display-flex margin-left-auto margin-right-0\" data-carousel-id=\"image-carousel-slider-carousel-6a8dc55763854\">\n\t\t\t\t<button class=\"hds-carousel-nav-arrow hds-carousel-arrow-prev\"><br \/>\n\t\t\t\t\t<svg version=\"1.1\" x=\"0px\" y=\"0px\" width=\"9px\" height=\"9px\" viewBox=\"0 0 9 9\"><path class=\"st0\" d=\"M3.5,4.5l3.7-3.6L6.3,0L1.8,4.5L6.3,9l0.9-0.9L3.5,4.5z\"><\/path><\/svg><br \/>\n\t\t\t\t<\/button><br \/>\n\t\t\t\t\t\t\t<button class=\"hds-carousel-nav-arrow hds-carousel-arrow-next margin-right-0\"><br \/>\n\t\t\t\t\t<svg version=\"1.1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" x=\"0px\" y=\"0px\" width=\"9px\" height=\"9px\" viewBox=\"0 0 9 9\"><path class=\"st0\" d=\"M5.5,4.5L1.8,8.1L2.7,9l4.5-4.5L2.7,0L1.8,0.9L5.5,4.5z\"><\/path><\/svg><br \/>\n\t\t\t\t<\/button>\n\t\t\t<\/div>\n<\/p>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\">X-rays are critical for the study of galaxies, revealing unique and important information about these cosmic building blocks. For example, Chandra exposes gas that has been superheated to millions of degrees by winds from massive stars, the outflows from supermassive black holes, and the debris from exploded stars. These are key sources of elements in our bodies, in the air we breathe, and the planet we live on. Chandra also sees some of the hottest and most energetic galactic phenomena in the universe, forming a more complete picture of how galaxies live, interact, and evolve when combined with data from other types of light and telescopes.<\/p>\n<h2 class=\"wp-block-heading\"><strong>Spiral and star-forming engines<\/strong><\/h2>\n<p class=\"wp-block-paragraph\">Face-on spiral galaxies like Messier 33 and NGC 3938 offer unobstructed views of places where energetic pairs of stars and cosmic explosions live along spiral arms. Barred spirals like NGC 1672 and NGC 1385 show how central bar-shaped collections of stars, gas, and dust funnel fuel inward to ignite bursts of star formation. NGC 4725 reveals how star formation can be triggered by a previous collision with another galaxy. Meanwhile, edge-on views of NGC 4631 (the Whale Galaxy) and the starburst Messier 82 (the Cigar Galaxy) showcase giant halos and superwinds of million-degree gas driven thousands of light-years into space by intense explosions of stars, enriching surrounding intergalactic space with vital elements.<\/p>\n<h2 class=\"wp-block-heading\"><strong>Active galactic nuclei, black hole outflows<\/strong><\/h2>\n<p class=\"wp-block-paragraph\">Powerful, growing black holes in the cores of their host galaxies, known as active galactic nuclei, send energy outward in outbursts and jets that impact entire galaxies. In Centaurus A, Chandra and IXPE data expose a high-energy particle jet blasting tens of thousands of light-years into space from its central engine. In Messier 106, jets from the supermassive black hole heat surrounding gas to create spiral arms that are different from those typically found in spiral galaxies. Meanwhile, the iconic Sombrero Galaxy (Messier 104) highlights a supermassive black hole embedded in a colossal stellar bulge, where Chandra\u2019s X-rays map a diffuse halo of million-degree gas and hot stellar remnants surrounding its sweeping dust lanes.<\/p>\n<h2 class=\"wp-block-heading\"><strong>Collisions, mergers, cosmic disruptions<\/strong><\/h2>\n<p class=\"wp-block-paragraph\">The gallery also showcases galaxies undergoing extreme gravitational transformations. A direct impact in Arp 143 acts like a cosmic bullseye, creating an expanding ring galaxy and triggering waves of star birth. Violent mergers, such as NGC 3256 and the dust-shrouded starburst II Zw 096, reveal the kind of chaotic galaxy collisions that dominated the early universe and offer a preview of the Milky Way\u2019s distant future merger with nearby galaxy Andromeda. NGC 1569 acts as a local laboratory for studying early universe starbursts, NGC 660 showcases a rare \u201cpolar ring\u201d galaxy where a ring of stars orbits over its poles, and Messier 90 shows a spiral galaxy plowing through the Virgo Cluster, having its star-forming gas violently stripped away.<\/p>\n<p class=\"wp-block-paragraph\">NASA\u2019s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory\u2019s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.<\/p>\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/chandra.si.edu\/photo\/2026\/galaxies\/\" rel=\"noopener\">Read more from NASA\u2019s Chandra X-ray Observatory<\/a><\/p>\n<p class=\"wp-block-paragraph\">To learn more about Chandra, visit<\/p>\n<p class=\"has-text-align-center wp-block-paragraph\"><a href=\"https:\/\/nasa.gov\/chandra\" rel=\"noopener\">https:\/\/nasa.gov\/chandra<\/a><\/p>\n<div id=\"\" class=\"hds-about-the-author nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-6 hds-module hds-module-full alignfull wp-block-nasa-blocks-about-the-author\">\n<div class=\"grid-row grid-container maxw-widescreen padding-x-0 border-top-1px border-color-carbon-black padding-top-3\">\n<div class=\"margin-bottom-4\">\n<h3 class=\"heading-14\">About the Author<\/h3>\n<\/div>\n<\/div>\n<div class=\"grid-row grid-container padding-x-0 maxw-widescreen\">\n<div class=\"grid-col-12 desktop:grid-col-6 desktop:padding-right-9\">\n<div class=\"grid-row\">\n<div class=\"hds-author-thumbnail mobile:circle-6 mobile:maxw-6 circle-card maxw-card thumbnail margin-right-2 desktop:margin-right-5\"><\/div>\n<div class=\"grid-col\">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-29 line-height-sm\">Megan Watzke<\/h2>\n<\/div>\n<div class=\"padding-y-2\"><\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"desktop:grid-col-6 desktop:padding-right-9\">\n<p class=\"margin-top-0\">\n<\/div>\n<\/div>\n<\/div>\n<div id=\"\" class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 nasa_template_article_c hds-module hds-module-full alignfull wp-block-nasa-blocks-credits-and-details\">\n<section class=\"padding-x-0 padding-top-5 padding-bottom-2 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"grid-row grid-container maxw-widescreen padding-0\">\n<div class=\"grid-col-12 desktop:grid-col-2 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black\">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Share<\/h2>\n<\/p>\n<\/div>\n<div class=\"padding-bottom-2\">\n<ul class=\"social-icons social-icons-round\">\n<li class=\"social-icon social-icon-x\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/x.com\/intent\/tweet?via=NASA&#038;text=Galactic%20Gems%20Glisten%20in%20New%20Gallery%20From%20NASA%E2%80%99s%20Chandra&#038;%23038;url=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fchandra%2Fgalactic-gems-glisten-in-new-gallery-from-nasas-chandra%2F\" aria-label=\"Share on X.\"><br \/>\n\t\t\t\t\t\t\t\t<svg width=\"1200\" height=\"1227\" viewBox=\"0 0 1200 1227\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><path d=\"M714.163 519.284L1160.89 0H1055.03L667.137 450.887L357.328 0H0L468.492 681.821L0 1226.37H105.866L515.491 750.218L842.672 1226.37H1200L714.137 519.284H714.163ZM569.165 687.828L521.697 619.934L144.011 79.6944H306.615L611.412 515.685L658.88 583.579L1055.08 1150.3H892.476L569.165 687.854V687.828Z\" fill=\"white\"\/><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<li class=\"social-icon social-icon-facebook\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/www.facebook.com\/sharer.php?u=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fchandra%2Fgalactic-gems-glisten-in-new-gallery-from-nasas-chandra%2F\" aria-label=\"Share on Facebook.\" rel=\"noopener\"><br \/>\n\t\t\t\t\t\t\t\t<svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewBox=\"0 0 24 24\" aria-hidden=\"true\"><path d=\"M9 8h-3v4h3v12h5v-12h3.642l.358-4h-4v-1.667c0-.955.192-1.333 1.115-1.333h2.885v-5h-3.808c-3.596 0-5.192 1.583-5.192 4.615v3.385z\"\/><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<li class=\"social-icon social-icon-linkedin\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/www.linkedin.com\/shareArticle?mini=true&#038;url=https%3A%2F%2Fscience.nasa.gov%2Fmissions%2Fchandra%2Fgalactic-gems-glisten-in-new-gallery-from-nasas-chandra%2F\" aria-label=\"Share on LinkedIn.\" rel=\"noopener\"><br \/>\n\t\t\t\t\t\t\t\t<svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewBox=\"0 0 24 24\" aria-hidden=\"true\"><path d=\"M4.98 3.5c0 1.381-1.11 2.5-2.48 2.5s-2.48-1.119-2.48-2.5c0-1.38 1.11-2.5 2.48-2.5s2.48 1.12 2.48 2.5zm.02 4.5h-5v16h5v-16zm7.982 0h-4.968v16h4.969v-8.399c0-4.67 6.029-5.052 6.029 0v8.399h4.988v-10.131c0-7.88-8.922-7.593-11.018-3.714v-2.155z\"\/><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<li class=\"social-icon social-icon-rss\">\n\t\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/feed\/\" aria-label=\"Subscribe to RSS feed.\"><br \/>\n\t\t\t\t\t\t\t\t<svg xmlns=\"http:\/\/www.w3.org\/2000\/svg\" viewBox=\"0 0 800 800\" aria-hidden=\"true\"><path d=\"M493 652H392c0-134-111-244-244-244V307c189 0 345 156 345 345zm71 0c0-228-188-416-416-416V132c285 0 520 235 520 520z\"\/><circle cx=\"219\" cy=\"581\" r=\"71\"\/><\/svg><br \/>\n\t\t\t\t\t\t\t<\/a>\n\t\t\t\t\t\t<\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 desktop:grid-col-5 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black\">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Details<\/h2>\n<\/p>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Last Updated<\/div>\n<\/p>\n<\/div>\n<div class=\"grid-col-8\">Aug 25, 2026<\/div>\n<\/p>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Editor<\/div>\n<\/div>\n<div class=\"grid-col-8\">Lee Mohon<\/div>\n<\/div>\n<div class=\"grid-row margin-bottom-3\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Contact<\/div>\n<\/div>\n<div class=\"grid-col-8\">\n<div class=\"margin-bottom-3\">\n<div>Megan Watzke<\/div>\n<div><a href=\"mailto:mwatzke@cfa.harvard.edu\">mwatzke@cfa.harvard.edu<\/a><\/div>\n<\/div>\n<div class=\"margin-bottom-3\">\n<div>Joel Wallace<\/div>\n<div><a href=\"mailto:joel.w.wallace@nasa.gov\">joel.w.wallace@nasa.gov<\/a><\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-row\">\n<div class=\"grid-col-4\">\n<div class=\"subheading\">Location<\/div>\n<\/div>\n<div class=\"grid-col-8\">Marshall Space Flight Center<\/div>\n<\/div>\n<\/div>\n<\/div>\n<div class=\"grid-col-12 desktop:grid-col-5 padding-right-4 margin-bottom-5 desktop:margin-bottom-0\">\n<div class=\"padding-top-3 border-top-1px border-color-carbon-black \">\n<div class=\"margin-bottom-2\">\n<h2 class=\"heading-14\">Related Terms<\/h2>\n<\/div>\n<ul class=\"article-tags\">\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/mission\/chandra\" rel=\"noopener\">Chandra X-Ray Observatory<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/active-galaxies\/\" rel=\"noopener\">Active Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/astrophysics\/\" rel=\"noopener\">Astrophysics<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/elliptical-galaxies\/\" rel=\"noopener\">Elliptical Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/galaxies\/\" rel=\"noopener\">Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/science-research\/astrophysics\/galaxies-stars-black-holes-research\/\" rel=\"noopener\">Galaxies, Stars, &#038; Black Holes Research<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/galaxy-mergers\/\" rel=\"noopener\">Galaxy Mergers<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/interacting-galaxies\/\" rel=\"noopener\">Interacting Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/irregular-galaxies\/\" rel=\"noopener\">Irregular Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/centers-and-facilities\/marshall\/marshall-science-research-and-projects\/marshall-astrophysics\/\" rel=\"noopener\">Marshall Astrophysics<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/www.nasa.gov\/marshall-space-flight-center\/\" rel=\"noopener\">Marshall Space Flight Center<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/category\/universe\/galaxies\/spiral-galaxies\/\" rel=\"noopener\">Spiral Galaxies<\/a><\/li>\n<li class=\"article-tag\"><a href=\"https:\/\/science.nasa.gov\/universe\/\" rel=\"noopener\">The Universe<\/a><\/li>\n<\/ul>\n<\/div>\n<\/div>\n<\/div>\n<\/section>\n<\/div>\n<div id=\"\" class=\"nasa-gb-align-full width-full maxw-full padding-x-3 padding-y-0 hds-module hds-module-full alignfull wp-block-nasa-blocks-related-articles\">\n<section class=\"hds-related-articles padding-x-0 padding-y-3 desktop:padding-top-7 desktop:padding-bottom-9\">\n<div class=\"w-100 grid-row grid-container maxw-widescreen padding-0 text-align-left\">\n<div class=\"margin-bottom-4\">\n<h2 style=\"max-width: 100%;\" class=\"width-full w-full maxw-full\">Explore More<\/h2>\n<\/div>\n<\/div>\n<div class=\"grid-row grid-container maxw-widescreen padding-0\">\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/missions\/chandra\/nasa-telescopes-create-colorful-craft-from-nearby-nebula\/\" class=\"color-carbon-black\" rel=\"noopener\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"8249\" height=\"7282\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=8249&#038;h=7282&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-medium size-medium\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=8249&#038;h=7282&#038;fit=crop&#038;crop=faces%2Cfocalpoint 8249w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=300&#038;h=265&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=768&#038;h=678&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=1024&#038;h=904&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=1536&#038;h=1356&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=2048&#038;h=1808&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=400&#038;h=353&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=600&#038;h=530&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=900&#038;h=794&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=1200&#038;h=1059&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/30dor_crop.jpg?w=2000&#038;h=1766&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 8249px) 100vw, 8249px\" \/><\/figure>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">4 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA Telescopes Create Colorful \u2018Craft\u2019 From Nearby Nebula<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t2 weeks ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/missions\/ixpe\/nasa-space-telescope-maps-magnetic-fields-of-lighthouse-pulsar\/\" class=\"color-carbon-black\" rel=\"noopener\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"3000\" height=\"2510\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=3000&#038;h=2510&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-medium size-medium\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=3000&#038;h=2510&#038;fit=crop&#038;crop=faces%2Cfocalpoint 3000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=300&#038;h=251&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=768&#038;h=643&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=1024&#038;h=857&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=1536&#038;h=1285&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=2048&#038;h=1713&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=400&#038;h=335&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=600&#038;h=502&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=900&#038;h=753&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=1200&#038;h=1004&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/ixpe\/lighthouse_ixpe_optical_radio_cxcxray.jpg?w=2000&#038;h=1673&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 3000px) 100vw, 3000px\" \/><\/figure>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">4 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA Space Telescope Maps Magnetic Fields of \u2018Lighthouse\u2019 Pulsar<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t2 months ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<div class=\"grid-col-12 desktop:grid-col-4 margin-bottom-4 desktop:margin-bottom-0 desktop:padding-right-3\">\n\t\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/missions\/chandra\/nasas-chandra-examines-milky-way-at-arms-length\/\" class=\"color-carbon-black\" rel=\"noopener\"><\/p>\n<div class=\"margin-bottom-2\">\n<div class=\"hds-cover-wrapper cover-hover-zoom bg-carbon-black minh-mobile\">\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"6000\" height=\"4000\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=6000&#038;h=4000&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-medium size-medium\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=6000&#038;h=4000&#038;fit=crop&#038;crop=faces%2Cfocalpoint 6000w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=300&#038;h=200&#038;fit=crop&#038;crop=faces%2Cfocalpoint 300w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=768&#038;h=512&#038;fit=crop&#038;crop=faces%2Cfocalpoint 768w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=1024&#038;h=683&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1024w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=1536&#038;h=1024&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1536w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=2048&#038;h=1365&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2048w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=400&#038;h=267&#038;fit=crop&#038;crop=faces%2Cfocalpoint 400w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=600&#038;h=400&#038;fit=crop&#038;crop=faces%2Cfocalpoint 600w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=900&#038;h=600&#038;fit=crop&#038;crop=faces%2Cfocalpoint 900w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=1200&#038;h=800&#038;fit=crop&#038;crop=faces%2Cfocalpoint 1200w, https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/arms_unlabeled.jpg?w=2000&#038;h=1333&#038;fit=crop&#038;crop=faces%2Cfocalpoint 2000w\" sizes=\"auto, (max-width: 6000px) 100vw, 6000px\" \/><\/figure>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"padding-right-0 desktop:padding-right-10\">\n<div class=\"subheading margin-bottom-1\">5 min read<\/div>\n<div class=\"margin-bottom-1\">\n<h3 class=\"related-article-title\">NASA\u2019s Chandra Examines Milky Way at Arms\u2019 Length<\/h3>\n<\/div>\n<div class=\"display-flex flex-align-center label related-article-label margin-bottom-1 color-carbon-60\">\n\t\t\t\t\t\t\t\t\t<span class=\"display-flex flex-align-center margin-right-2\"><br \/>\n\t\t\t\t\t\t\t\t\t\t<svg version=\"1.1\" class=\"square-2 margin-right-1\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\" xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" x=\"0px\" y=\"0px\" width=\"16px\" height=\"16px\" viewBox=\"0 0 16 16\" style=\"enable-background:new 0 0 16 16;\" xml:space=\"preserve\"><g><g><path d=\"M8,0C3.5,0-0.1,3.7,0,8.2C0.1,12.5,3.6,16,8,16c4.4,0,8-3.6,8-8C16,3.5,12.4,0,8,0z M8,15.2 C4,15.2,0.8,12,0.8,8C0.8,4,4,0.8,8,0.8c3.9,0,7.2,3.2,7.2,7.1C15.2,11.9,12,15.2,8,15.2z\"\/><path d=\"M5.6,12c0.8-0.8,1.6-1.6,2.4-2.4c0.8,0.8,1.6,1.6,2.4,2.4c0-2.7,0-5.3,0-8C8.8,4,7.2,4,5.6,4 C5.6,6.7,5.6,9.3,5.6,12z\"\/><\/g><\/g><\/svg><br \/>\n\t\t\t\t\t\t\t\t\t\t<span>Article<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<\/span><br \/>\n\t\t\t\t\t\t\t\t\t<span class=\"\"><br \/>\n\t\t\t\t\t\t\t\t\t\t2 months ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<p>\t\t\t\t\t\t<\/a>\n\t\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<\/section>\n<\/div>\n<div id=\"\" class=\"hds-topic-cards nasa-gb-align-full maxw-full width-full padding-y-6 padding-x-3 color-mode-dark hds-module hds-module-full alignfull wp-block-nasa-blocks-topic-cards\">\n<div class=\"grid-container grid-container-block-lg padding-x-0\">\n<div class=\"grid-row flex-align-center margin-bottom-3\">\n<div class=\"desktop:grid-col-8 margin-bottom-2 desktop:margin-bottom-0\">\n<div class=\"label color-carbon-60 margin-bottom-2\">Keep Exploring<\/div>\n<h2 class=\"heading-36 line-height-sm\">Discover More Topics From NASA<\/h2>\n<\/p>\n<\/div>\n<\/div>\n<div class=\"grid-row grid-gap-2 hds-topic-cards-wrapper\">\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/3d-resources\/chandra-x-ray-observatory\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<p class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Chandra X-ray Observatory<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"1920\" height=\"1080\" src=\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/cds\/3d\/resources\/model\/chandra-x-ray-observatory\/Chandra%20X-ray%20Observatory.png?w=1920&#038;h=1080&#038;%23038;fit=clip&#038;%23038;crop=faces%2Cfocalpoint\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/hubble\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<h3 class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>Hubble Space Telescope<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"1512\" height=\"1536\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?w=1512\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg 4031w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=295,300 295w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=768,780 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=1008,1024 1008w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=1512,1536 1512w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=2016,2048 2016w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=50,50 50w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=394,400 394w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=591,600 591w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=886,900 886w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=1181,1200 1181w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/07\/hubble-space-telescope-hst-6.jpg?resize=1969,2000 1969w\" sizes=\"auto, (max-width: 1512px) 100vw, 1512px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/james-webb-space-telescope\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<h3 class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>James Webb Space Telescope<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the\u2026<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"1536\" height=\"890\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp 3600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=300,174 300w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=768,445 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1024,593 1024w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1536,890 1536w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2048,1186 2048w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=400,232 400w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=600,348 600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=900,521 900w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=1200,695 1200w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/03\/main-image-star-forming-region-carina-nircam-final-5mb-1-jpeg.webp?resize=2000,1158 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a><br \/>\n\t\t\t\t\t<a href=\"https:\/\/science.nasa.gov\/mission\/ixpe\/\" class=\"mobile:grid-col-12 tablet:grid-col-6 desktop:grid-col-3 topic-card margin-bottom-4 desktop:margin-bottom-0\" rel=\"noopener\"><\/p>\n<div class=\"hds-topic-card hds-cover-wrapper cover-hover-zoom bg-carbon-black\">\n<div class=\"skrim-overlay skrim-overlay-dark skrim-left mobile-skrim-top padding-3 display-flex flex-align-end flex-justify-start z-200\">\n<div>\n<h3 class=\"hds-topic-card-heading heading-29 color-spacesuit-white line-height-sm margin-top-0 margin-bottom-1\">\n\t\t\t\t\t\t\t\t<span>IXPE<\/span><br \/>\n\t\t\t\t\t\t\t\t<svg viewBox=\"0 0 32 32\" fill=\"none\" xmlns=\"http:\/\/www.w3.org\/2000\/svg\"><circle class=\"color-nasa-red\" cx=\"16\" cy=\"16\" r=\"16\"><\/circle><path d=\"M8 16.956h12.604l-3.844 4.106 1.252 1.338L24 16l-5.988-6.4-1.252 1.338 3.844 4.106H8v1.912z\" class=\"color-spacesuit-white\"><\/path><\/svg><br \/>\n\t\t\t\t\t\t\t<\/h3>\n<p class=\"margin-bottom-0 margin-top-2 color-carbon-20-important\">The Imaging X-ray Polarimetry Explorer (IXPE) is NASA\u2019s first mission to study the polarization of X-rays.<\/p>\n<\/p>\n<\/div>\n<\/div>\n<figure class=\"hds-media-background  \"><img decoding=\"async\" width=\"1536\" height=\"864\" src=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?w=1536\" class=\"attachment-1536x1536 size-1536x1536\" alt=\"\" style=\"transform: scale(1); transform-origin: 50% 50%; object-position: 50% 50%; object-fit: cover;\" block_context=\"nasa-block\" loading=\"lazy\" srcset=\"https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp 4000w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=300,169 300w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=768,432 768w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=1024,576 1024w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=1536,864 1536w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=2048,1152 2048w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=400,225 400w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=600,338 600w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=900,506 900w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=1200,675 1200w, https:\/\/science.nasa.gov\/wp-content\/uploads\/2023\/06\/ixpe-003-jpg.webp?resize=2000,1125 2000w\" sizes=\"auto, (max-width: 1536px) 100vw, 1536px\" \/><\/figure>\n<\/p>\n<\/div>\n<p>\t\t\t<\/a>\n\t\t\t\t<\/div>\n<\/p>\n<\/div>\n<\/div>\n<p class=\"wp-block-paragraph\">\n","protected":false},"excerpt":{"rendered":"<p>Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]<\/p>\n","protected":false},"author":13,"featured_media":0,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"om_disable_all_campaigns":false,"_monsterinsights_skip_tracking":false,"_uf_show_specific_survey":0,"_uf_disable_surveys":false,"footnotes":""},"categories":[16543,15612,15670,15773,15757,16610,19395,15774,17143,15672,15673,15758,15638],"tags":[],"class_list":["post-519875","post","type-post","status-publish","format-standard","hentry","category-active-galaxies","category-astrophysics","category-chandra-x-ray-observatory","category-elliptical-galaxies","category-galaxies","category-galaxies-stars-black-holes-research","category-galaxy-mergers","category-interacting-galaxies","category-irregular-galaxies","category-marshall-astrophysics","category-marshall-space-flight-center","category-spiral-galaxies","category-the-universe"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO Pro 5.0.1 - aioseo.com -->\n\t<meta name=\"description\" content=\"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]\" \/>\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<meta name=\"author\" content=\"Guest authors\"\/>\n\t<meta name=\"google-site-verification\" content=\"1EIWGZ5FoylKQrO3pqls-2hXlDXKIP1lffdWZCVV0V4\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.vibewire.com.au\/?p=519875\" \/>\n\t<meta name=\"generator\" content=\"All in One SEO Pro (AIOSEO) 5.0.1\" \/>\n\t\t<meta property=\"og:locale\" content=\"en_US\" \/>\n\t\t<meta property=\"og:site_name\" content=\"VibeWire Magazine - Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine\" \/>\n\t\t<meta property=\"og:description\" content=\"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]\" \/>\n\t\t<meta property=\"og:url\" content=\"https:\/\/www.vibewire.com.au\/?p=519875\" \/>\n\t\t<meta property=\"article:published_time\" content=\"2026-08-25T16:13:49+00:00\" \/>\n\t\t<meta property=\"article:modified_time\" content=\"2026-08-25T16:13:49+00:00\" \/>\n\t\t<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n\t\t<meta name=\"twitter:site\" content=\"@VibewireCentral\" \/>\n\t\t<meta name=\"twitter:title\" content=\"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine\" \/>\n\t\t<meta name=\"twitter:description\" content=\"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]\" \/>\n\t\t<meta name=\"twitter:creator\" content=\"@VibewireCentral\" \/>\n\t\t<script type=\"application\/ld+json\" class=\"aioseo-schema\">\n\t\t\t{\"@context\":\"https:\\\/\\\/schema.org\",\"@graph\":[{\"@type\":\"BlogPosting\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#blogposting\",\"name\":\"Galactic Gems Glisten in New Gallery From NASA\\u2019s Chandra - VibeWire Magazine\",\"headline\":\"Galactic Gems Glisten in New Gallery From NASA\\u2019s Chandra\",\"author\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?author=13#author\"},\"publisher\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/#organization\"},\"image\":{\"@type\":\"ImageObject\",\"url\":\"https:\\\/\\\/assets.science.nasa.gov\\\/dynamicimage\\\/assets\\\/science\\\/missions\\\/chandra\\\/2026\\\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&%23038;fit=clip&%23038;crop=faces%2Cfocalpoint\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875\\\/#articleImage\"},\"datePublished\":\"2026-08-26T02:13:49+10:00\",\"dateModified\":\"2026-08-26T02:13:49+10:00\",\"inLanguage\":\"en-AU\",\"mainEntityOfPage\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#webpage\"},\"isPartOf\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#webpage\"},\"articleSection\":\"Active Galaxies, Astrophysics, Chandra X-Ray Observatory, Elliptical Galaxies, Galaxies, Galaxies, Stars, &amp; Black Holes Research, Galaxy Mergers, Interacting Galaxies, Irregular Galaxies, Marshall Astrophysics, Marshall Space Flight Center, Spiral Galaxies, The Universe\"},{\"@type\":\"BreadcrumbList\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#breadcrumblist\",\"itemListElement\":[{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au#listItem\",\"position\":1,\"name\":\"Home\",\"item\":\"https:\\\/\\\/www.vibewire.com.au\",\"nextItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?cat=15612#listItem\",\"name\":\"Astrophysics\"}},{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?cat=15612#listItem\",\"position\":2,\"name\":\"Astrophysics\",\"item\":\"https:\\\/\\\/www.vibewire.com.au\\\/?cat=15612\",\"nextItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#listItem\",\"name\":\"Galactic Gems Glisten in New Gallery From NASA\\u2019s Chandra\"},\"previousItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au#listItem\",\"name\":\"Home\"}},{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#listItem\",\"position\":3,\"name\":\"Galactic Gems Glisten in New Gallery From NASA\\u2019s Chandra\",\"previousItem\":{\"@type\":\"ListItem\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?cat=15612#listItem\",\"name\":\"Astrophysics\"}}]},{\"@type\":\"Organization\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/#organization\",\"name\":\"VibreWire Online\",\"description\":\"Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything\",\"url\":\"https:\\\/\\\/www.vibewire.com.au\\\/\",\"logo\":{\"@type\":\"ImageObject\",\"url\":\"https:\\\/\\\/www.vibewire.com.au\\\/wp-content\\\/uploads\\\/2024\\\/02\\\/Screenshot-2024-01-07-at-2.32.21\\u202fpm.png\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875\\\/#organizationLogo\",\"width\":1028,\"height\":930},\"image\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875\\\/#organizationLogo\"},\"sameAs\":[\"https:\\\/\\\/twitter.com\\\/VibewireCentral\"]},{\"@type\":\"Person\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?author=13#author\",\"url\":\"https:\\\/\\\/www.vibewire.com.au\\\/?author=13\",\"name\":\"Guest authors\",\"image\":{\"@type\":\"ImageObject\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#authorImage\",\"url\":\"https:\\\/\\\/secure.gravatar.com\\\/avatar\\\/764687183b9d2913837d7b543a5b43684d46e7eef4e1a9af4821624eb2bebbc0?s=96&d=mm&r=g\",\"width\":96,\"height\":96,\"caption\":\"Guest authors\"}},{\"@type\":\"WebPage\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#webpage\",\"url\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875\",\"name\":\"Galactic Gems Glisten in New Gallery From NASA\\u2019s Chandra - VibeWire Magazine\",\"description\":\"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\\u2026]\",\"inLanguage\":\"en-AU\",\"isPartOf\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/#website\"},\"breadcrumb\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?p=519875#breadcrumblist\"},\"author\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?author=13#author\"},\"creator\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/?author=13#author\"},\"datePublished\":\"2026-08-26T02:13:49+10:00\",\"dateModified\":\"2026-08-26T02:13:49+10:00\"},{\"@type\":\"WebSite\",\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/#website\",\"url\":\"https:\\\/\\\/www.vibewire.com.au\\\/\",\"name\":\"VibreWire Online\",\"description\":\"Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything\",\"inLanguage\":\"en-AU\",\"publisher\":{\"@id\":\"https:\\\/\\\/www.vibewire.com.au\\\/#organization\"}}]}\n\t\t<\/script>\n\t\t<!-- All in One SEO Pro -->\r\n\t\t<title>Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine<\/title>\n\n","aioseo_head_json":{"title":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine","description":"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]","canonical_url":"https:\/\/www.vibewire.com.au\/?p=519875","robots":"max-image-preview:large","keywords":"","webmasterTools":{"google-site-verification":"1EIWGZ5FoylKQrO3pqls-2hXlDXKIP1lffdWZCVV0V4","miscellaneous":""},"schema":{"@context":"https:\/\/schema.org","@graph":[{"@type":"BlogPosting","@id":"https:\/\/www.vibewire.com.au\/?p=519875#blogposting","name":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine","headline":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra","author":{"@id":"https:\/\/www.vibewire.com.au\/?author=13#author"},"publisher":{"@id":"https:\/\/www.vibewire.com.au\/#organization"},"image":{"@type":"ImageObject","url":"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/missions\/chandra\/2026\/galaxies_ngc4631.jpg?w=4336&#038;h=2794&%23038;fit=clip&%23038;crop=faces%2Cfocalpoint","@id":"https:\/\/www.vibewire.com.au\/?p=519875\/#articleImage"},"datePublished":"2026-08-26T02:13:49+10:00","dateModified":"2026-08-26T02:13:49+10:00","inLanguage":"en-AU","mainEntityOfPage":{"@id":"https:\/\/www.vibewire.com.au\/?p=519875#webpage"},"isPartOf":{"@id":"https:\/\/www.vibewire.com.au\/?p=519875#webpage"},"articleSection":"Active Galaxies, Astrophysics, Chandra X-Ray Observatory, Elliptical Galaxies, Galaxies, Galaxies, Stars, &amp; Black Holes Research, Galaxy Mergers, Interacting Galaxies, Irregular Galaxies, Marshall Astrophysics, Marshall Space Flight Center, Spiral Galaxies, The Universe"},{"@type":"BreadcrumbList","@id":"https:\/\/www.vibewire.com.au\/?p=519875#breadcrumblist","itemListElement":[{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au#listItem","position":1,"name":"Home","item":"https:\/\/www.vibewire.com.au","nextItem":{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au\/?cat=15612#listItem","name":"Astrophysics"}},{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au\/?cat=15612#listItem","position":2,"name":"Astrophysics","item":"https:\/\/www.vibewire.com.au\/?cat=15612","nextItem":{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au\/?p=519875#listItem","name":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra"},"previousItem":{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au#listItem","name":"Home"}},{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au\/?p=519875#listItem","position":3,"name":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra","previousItem":{"@type":"ListItem","@id":"https:\/\/www.vibewire.com.au\/?cat=15612#listItem","name":"Astrophysics"}}]},{"@type":"Organization","@id":"https:\/\/www.vibewire.com.au\/#organization","name":"VibreWire Online","description":"Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything","url":"https:\/\/www.vibewire.com.au\/","logo":{"@type":"ImageObject","url":"https:\/\/www.vibewire.com.au\/wp-content\/uploads\/2024\/02\/Screenshot-2024-01-07-at-2.32.21\u202fpm.png","@id":"https:\/\/www.vibewire.com.au\/?p=519875\/#organizationLogo","width":1028,"height":930},"image":{"@id":"https:\/\/www.vibewire.com.au\/?p=519875\/#organizationLogo"},"sameAs":["https:\/\/twitter.com\/VibewireCentral"]},{"@type":"Person","@id":"https:\/\/www.vibewire.com.au\/?author=13#author","url":"https:\/\/www.vibewire.com.au\/?author=13","name":"Guest authors","image":{"@type":"ImageObject","@id":"https:\/\/www.vibewire.com.au\/?p=519875#authorImage","url":"https:\/\/secure.gravatar.com\/avatar\/764687183b9d2913837d7b543a5b43684d46e7eef4e1a9af4821624eb2bebbc0?s=96&d=mm&r=g","width":96,"height":96,"caption":"Guest authors"}},{"@type":"WebPage","@id":"https:\/\/www.vibewire.com.au\/?p=519875#webpage","url":"https:\/\/www.vibewire.com.au\/?p=519875","name":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine","description":"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]","inLanguage":"en-AU","isPartOf":{"@id":"https:\/\/www.vibewire.com.au\/#website"},"breadcrumb":{"@id":"https:\/\/www.vibewire.com.au\/?p=519875#breadcrumblist"},"author":{"@id":"https:\/\/www.vibewire.com.au\/?author=13#author"},"creator":{"@id":"https:\/\/www.vibewire.com.au\/?author=13#author"},"datePublished":"2026-08-26T02:13:49+10:00","dateModified":"2026-08-26T02:13:49+10:00"},{"@type":"WebSite","@id":"https:\/\/www.vibewire.com.au\/#website","url":"https:\/\/www.vibewire.com.au\/","name":"VibreWire Online","description":"Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything","inLanguage":"en-AU","publisher":{"@id":"https:\/\/www.vibewire.com.au\/#organization"}}]},"og:locale":"en_US","og:site_name":"VibeWire Magazine - Your Alternate News Source for Transport, Politics, UFO, Paranormal, Anything","og:type":"article","og:title":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine","og:description":"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]","og:url":"https:\/\/www.vibewire.com.au\/?p=519875","article:published_time":"2026-08-25T16:13:49+00:00","article:modified_time":"2026-08-25T16:13:49+00:00","twitter:card":"summary_large_image","twitter:site":"@VibewireCentral","twitter:title":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra - VibeWire Magazine","twitter:description":"Galaxies are like cosmic gems, each with characteristics including size and shape that make them distinct. A new gallery released today from NASA\u2019s Chandra X-ray Observatory and other telescopes displays a collection of galactic images that showcase this variety. Astronomers put galaxies into three main categories: spirals like our own Milky Way with arms emanating [\u2026]","twitter:creator":"@VibewireCentral"},"aioseo_meta_data":{"post_id":"519875","title":null,"description":null,"keywords":null,"keyphrases":null,"primary_term":null,"canonical_url":null,"og_title":null,"og_description":null,"og_object_type":"default","og_image_type":"default","og_image_url":null,"og_image_width":null,"og_image_height":null,"og_image_custom_url":null,"og_image_custom_fields":null,"og_video":null,"og_custom_url":null,"og_article_section":null,"og_article_tags":null,"twitter_use_og":false,"twitter_card":"default","twitter_image_type":"default","twitter_image_url":null,"twitter_image_custom_url":null,"twitter_image_custom_fields":null,"twitter_title":null,"twitter_description":null,"schema":{"blockGraphs":[],"customGraphs":[],"default":{"data":{"Article":[],"Course":[],"Dataset":[],"FAQPage":[],"Movie":[],"Person":[],"Product":[],"ProductReview":[],"Car":[],"Recipe":[],"Service":[],"SoftwareApplication":[],"WebPage":[]},"graphName":"","isEnabled":true},"graphs":[]},"schema_type":"default","schema_type_options":null,"pillar_content":false,"robots_default":true,"robots_noindex":false,"robots_noarchive":false,"robots_nosnippet":false,"robots_nofollow":false,"robots_noimageindex":false,"robots_noodp":false,"robots_notranslate":false,"robots_max_snippet":null,"robots_max_videopreview":null,"robots_max_imagepreview":"large","priority":null,"frequency":null,"local_seo":null,"seo_analyzer_scan_date":"2026-08-25 17:49:28","breadcrumb_settings":null,"limit_modified_date":false,"open_ai":null,"ai":null,"created":"2026-08-25 17:49:16","updated":"2026-08-25 17:49:28","focus_keyword":null,"additional_keywords":null,"truseo_locale":null},"aioseo_breadcrumb":"<div class=\"aioseo-breadcrumbs\"><span class=\"aioseo-breadcrumb\">\n\t<a href=\"https:\/\/www.vibewire.com.au\" title=\"Home\">Home<\/a>\n<\/span><span class=\"aioseo-breadcrumb-separator\">&raquo;<\/span><span class=\"aioseo-breadcrumb\">\n\t<a href=\"https:\/\/www.vibewire.com.au\/?cat=15612\" title=\"Astrophysics\">Astrophysics<\/a>\n<\/span><span class=\"aioseo-breadcrumb-separator\">&raquo;<\/span><span class=\"aioseo-breadcrumb\">\n\tGalactic Gems Glisten in New Gallery From NASA\u2019s Chandra\n<\/span><\/div>","aioseo_breadcrumb_json":[{"label":"Home","link":"https:\/\/www.vibewire.com.au"},{"label":"Astrophysics","link":"https:\/\/www.vibewire.com.au\/?cat=15612"},{"label":"Galactic Gems Glisten in New Gallery From NASA\u2019s Chandra","link":"https:\/\/www.vibewire.com.au\/?p=519875"}],"_links":{"self":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/519875","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/users\/13"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=519875"}],"version-history":[{"count":1,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/519875\/revisions"}],"predecessor-version":[{"id":519876,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=\/wp\/v2\/posts\/519875\/revisions\/519876"}],"wp:attachment":[{"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=519875"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=519875"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vibewire.com.au\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=519875"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}